OS039-07
Observing rain layers, diurnal warm layers, and their impacts in tropical oceans
Observing rain layers, diurnal warm layers, and their impacts in tropical oceans
Monday, 14 December 2020: 10:18
Virtual
Abstract:
Near surface stratification of the ocean by rain and solar radiation absorption limits the depth penetration of ocean mixing and amplifies the surface variability of ocean temperature, salinity, and air-sea fluxes. We review investigations of these coupled processes from recent field campaigns across the tropical Indian and Pacific Oceans: PISTON 2018-2019, SPURS-2 2016-2017, DYNAMO 2011. When diurnal warm layers are present, the diurnal variations in latent, sensible, and buoyancy fluxes into the atmosphere are amplified due to warm SST and atmospheric boundary layer drying. When stable "rain layers" exist at the surface following precipitation, air-sea fluxes are also enhanced by rain-cooled SST because the atmospheric boundary layer cools considerably more than the ocean during rain and also often dries. We discuss in-situ, radar-, and satellite-based strategies for measuring rain layers, diurnal warm layers, and their impacts on the upper ocean and lower atmosphere. Using only the surface wind speed, surface buoyancy flux, and Monin-Obukhov similarity theory we derived estimates of ocean stable layer depth and the maximum surface wind speed for which ocean stratification should persist for a given surface buoyancy flux. During the equatorial DYNAMO experiment, these estimates accurately diagnosed 36 out of 44 observed stratification events (88% success rate) and also accurately diagnosed the wind limits of these events. We assess the performance of these techniques during off-equatorial field campaigns: SPURS-2 and PISTON. The success of this stable layer detection method suggests a means to determine the presence of stable near-surface rain layers and diurnal warm layers in the ocean from only surface measurements in the atmosphere: wind, rain rate, and air-sea heat fluxes.